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Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model - MaRDI portal

Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model

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Publication:4905526

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DOI10.1051/0004-6361/201014731zbMath1260.85027arXiv1007.4961OpenAlexW2116152809WikidataQ63644413 ScholiaQ63644413MaRDI QIDQ4905526

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Publication date: 19 February 2013

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1007.4961

zbMATH Keywords

stars: neutron X-rays: binaries

Mathematics Subject Classification ID

Three-body problems (70F07) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar dynamics (85A05)

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